Incorporating Morphological Types into Semi-analytic Schemes for Galaxy Formation

Simple item page
dc.creatorBaugh, C. M.
dc.date1995-09-13
dc.date.accessioned2026-07-07T02:20:10Z
dc.date.available2026-07-07T02:20:10Z
dc.descriptionWe test the hypothesis that elliptical galaxies are formed by violent mergers in a universe with hierarchical structure formation. Within the framework of a semi-analytic scheme for galaxy formation, we predict the distribution of morphological types with redshift and compare the colours of elliptical galaxies in different environments.
dc.description4 pages of uuencoded compressed PostScript; to appear in the proceedings of the 11th IAP meeting, "The interplay between massive star formation, the ISM and galaxy evolution"
dc.identifierhttps://arxiv.org/abs/astro-ph/9509069
dc.identifierhttp://arxiv.org/abs/astro-ph/9509069
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10129
dc.subjectAstrophysics
dc.titleIncorporating Morphological Types into Semi-analytic Schemes for Galaxy Formation
dc.typetext

Files

Collections

arXiv